Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Bernardis, PD"'
Autor:
Collaboration, P, Akrami, Y, Ashdown, M, Aumont, J, Baccigalupi, C, Ballardini, M, Banday, AJ, Barreiro, RB, Bartolo, N, Basak, S, Benabed, K, Bernard, J-P, Bersanelli, M, Bielewicz, P, Bond, JR, Borrill, J, Bouchet, FR, Burigana, C, Calabrese, E, Cardoso, J-F, Casaponsa, B, Chiang, HC, Combet, C, Contreras, D, Crill, BP, Cuttaia, F, Bernardis, PD, Rosa, AD, Zotti, GD, Delabrouille, J, Valentino, ED, Diego, JM, Doré, O, Douspis, M, Dupac, X, Enßlin, TA, Eriksen, HK, Fernandez-Cobos, R, Finelli, F, Frailis, M, Franceschi, E, Frolov, A, Galeotta, S, Galli, S, Ganga, K, Génova-Santos, RT, Gerbino, M, González-Nuevo, J, Górski, KM, Gruppuso, A, Gudmundsson, JE, Handley, W, Herranz, D, Hivon, E, Huang, Z, Jaffe, AH, Jones, WC, Keihänen, E, Keskitalo, R, Kiiveri, K, Kim, J, Kisner, TS, Krachmalnicoff, N, Kunz, M, Kurki-Suonio, H, Lamarre, J-M, Lattanzi, M, Lawrence, CR, Jeune, ML, Levrier, F, Liguori, M, Lilje, PB, Lindholm, V, López-Caniego, M, Macías-Pérez, JF, Maino, D, Mandolesi, N, Marcos-Caballero, A, Maris, M, Martin, PG, Martínez-González, E, Matarrese, S, Mauri, N, McEwen, JD, Mennella, A, Migliaccio, M, Molinari, D, Moneti, A, Montier, L, Morgante, G, Moss, A, Natoli, P, Pagano, L, Paoletti, D, Perrotta, F, Pettorino, V, Piacentini, F, Polenta, G, Rachen, JP, Reinecke, M, Remazeilles, M, Renzi, A, Rocha, G, Rosset, C, Rubiño-Martín, JA, Ruiz-Granados, B, Salvati, L, Savelainen, M, Scott, D, Sirignano, C, Sirri, G, Spencer, LD, Sullivan, RM, Sunyaev, R, Suur-Uski, A-S, Tauber, JA, Tavagnacco, D, Tenti, M, Toffolatti, L, Tomasi, M, Trombetti, T, Valiviita, J, Tent, BV, Vielva, P, Villa, F, Vittorio, N, Wehus, IK, Zacchei, A, Zonca, A
The largest temperature anisotropy in the cosmic microwave background (CMB) is the dipole, which has been measured with increasing accuracy for more than three decades, particularly with the Planck satellite. The simplest interpretation of the dipole
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1032::3714810881c4df27c78c1abeb7527baa
http://hdl.handle.net/10044/1/82829
http://hdl.handle.net/10044/1/82829
Autor:
Collaboration, P, Akrami, Y, Andersen, KJ, Ashdown, M, Baccigalupi, C, Ballardini, M, Banday, AJ, Barreiro, RB, Bartolo, N, Basak, S, Benabed, K, Bernard, J-P, Bersanelli, M, Bielewicz, P, Bond, JR, Borrill, J, Burigana, C, Butler, RC, Calabrese, E, Casaponsa, B, Chiang, HC, Colombo, LPL, Combet, C, Crill, BP, Cuttaia, F, Bernardis, PD, Rosa, AD, Zotti, GD, Delabrouille, J, Valentino, ED, Diego, JM, Doré, O, Douspis, M, Dupac, X, Eriksen, HK, Fernandez-Cobos, R, Finelli, F, Frailis, M, Fraisse, AA, Franceschi, E, Frolov, A, Galeotta, S, Galli, S, Ganga, K, Gerbino, M, Ghosh, T, González-Nuevo, J, Górski, KM, Gruppuso, A, Gudmundsson, JE, Handley, W, Helou, G, Herranz, D, Hildebrandt, SR, Hivon, E, Huang, Z, Jaffe, AH, Jones, WC, Keihänen, E, Keskitalo, R, Kiiveri, K, Kim, J, Kisner, TS, Krachmalnicoff, N, Kunz, M, Kurki-Suonio, H, Lasenby, A, Lattanzi, M, Lawrence, CR, Jeune, ML, Levrier, F, Liguori, M, Lilje, PB, Lilley, M, Lindholm, V, López-Caniego, M, Lubin, PM, Macías-Pérez, JF, Maino, D, Mandolesi, N, Marcos-Caballero, A, Maris, M, Martin, PG, Martínez-González, E, Matarrese, S, Mauri, N, McEwen, JD, Meinhold, PR, Mennella, A, Migliaccio, M, Mitra, S, Molinari, D, Montier, L, Morgante, G, Moss, A, Natoli, P, Paoletti, D, Partridge, B, Patanchon, G, Pearson, D, Pearson, TJ, Perrotta, F, Piacentini, F, Polenta, G, Rachen, JP, Reinecke, M, Remazeilles, M, Renzi, A, Rocha, G, Rosset, C, Roudier, G, Rubiño-Martín, JA, Ruiz-Granados, B, Salvati, L, Savelainen, M, Scott, D, Sirignano, C, Sirri, G, Spencer, LD, Suur-Uski, A-S, Svalheim, TL, Tauber, JA, Tavagnacco, D, Tenti, M, Terenzi, L, Thommesen, H, Toffolatti, L, Tomasi, M, Tristram, M, Trombetti, T, Valiviita, J, Tent, BV, Vielva, P, Villa, F, Vittorio, N, Wandelt, BD, Wehus, IK, Zacchei, A, Zonca, A
We present the NPIPE processing pipeline, which produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency Instrument (LFI) and High Frequency Instrument (HFI) using high-performance computers. NPIPE re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1032::ae767dedda6f2abbc08ae708bb80b65a
http://hdl.handle.net/10044/1/82462
http://hdl.handle.net/10044/1/82462
Autor:
Collaboration, P, Aghanim, N, Akrami, Y, Alves, MIR, Ashdown, M, Aumont, J, Baccigalupi, C, Ballardini, M, Banday, AJ, Barreiro, RB, Bartolo, N, Basak, S, Benabed, K, Bernard, J-P, Bersanelli, M, Bielewicz, P, Bock, JJ, Bond, JR, Borrill, J, Bouchet, FR, Boulanger, F, Bracco, A, Bucher, M, Burigana, C, Calabrese, E, Cardoso, J-F, Carron, J, Chary, R-R, Chiang, HC, Colombo, LPL, Combet, C, Crill, BP, Cuttaia, F, Bernardis, PD, Zotti, GD, Delabrouille, J, Delouis, J-M, Valentino, ED, Dickinson, C, Diego, JM, Doré, O, Douspis, M, Ducout, A, Dupac, X, Efstathiou, G, Elsner, F, Enßlin, TA, Eriksen, HK, Fantaye, Y, Fernandez-Cobos, R, Ferrière, K, Forastieri, F, Frailis, M, Fraisse, AA, Franceschi, E, Frolov, A, Galeotta, S, Galli, S, Ganga, K, Génova-Santos, RT, Gerbino, M, Ghosh, T, González-Nuevo, J, Górski, KM, Gratton, S, Green, G, Gruppuso, A, Gudmundsson, JE, Guillet, V, Handley, W, Hansen, FK, Helou, G, Herranz, D, Hivon, E, Huang, Z, Jaffe, AH, Jones, WC, Keihänen, E, Keskitalo, R, Kiiveri, K, Kim, J, Krachmalnicoff, N, Kunz, M, Kurki-Suonio, H, Lagache, G, Lamarre, J-M, Lasenby, A, Lattanzi, M, Lawrence, CR, Jeune, ML, Levrier, F, Liguori, M, Lilje, PB, Lindholm, V, López-Caniego, M, Lubin, PM, Ma, Y-Z, Macías-Pérez, JF, Maggio, G, Maino, D, Mandolesi, N, Mangilli, A, Marcos-Caballero, A, Maris, M, Martin, PG, Martínez-González, E, Matarrese, S, Mauri, N, McEwen, JD, Melchiorri, A, Mennella, A, Migliaccio, M, Miville-Deschênes, M-A, Molinari, D, Moneti, A, Montier, L, Morgante, G, Moss, A, Natoli, P, Pagano, L, Paoletti, D, Patanchon, G, Perrotta, F, Pettorino, V, Piacentini, F, Polastri, L, Polenta, G, Puget, J-L, Rachen, JP, Reinecke, M, Remazeilles, M, Renzi, A, Ristorcelli, I, Rocha, G, Rosset, C, Roudier, G, Rubiño-Martín, JA, Ruiz-Granados, B, Salvati, L, Sandri, M, Savelainen, M, Scott, D, Sirignano, C, Sunyaev, R, Suur-Uski, A-S, Tauber, JA, Tavagnacco, D, Tenti, M, Toffolatti, L, Tomasi, M, Trombetti, T, Valiviita, J, Tent, BV, Vielva, P, Villa, F, Vittorio, N, Wandelt, BD, Wehus, IK, Zacchei, A, Zonca, A
Publikováno v:
Collaboration, P; Aghanim, N; Akrami, Y; Alves, MIR; Ashdown, M; Aumont, J; et al.(2018). Planck 2018 results. XII. Galactic astrophysics using polarized dust emission. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/1mj6w9ns
We present 353 GHz full-sky maps of the polarization fraction $p$, angle $\psi$, and dispersion of angles $S$ of Galactic dust thermal emission produced from the 2018 release of Planck data. We confirm that the mean and maximum of $p$ decrease with i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::eb22e1f2042c1c9f6138605db71dde59
http://www.escholarship.org/uc/item/1mj6w9ns
http://www.escholarship.org/uc/item/1mj6w9ns
Autor:
Collaboration, P, Ade, PAR, Aghanim, N, Arnaud, M, Aumont, J, Baccigalupi, C, Banday, AJ, Barreiro, RB, Bartolo, N, Battaner, E, Benabed, K, Benoit-Lévy, A, Bernard, J-P, Bersanelli, M, Bielewicz, P, Bonaldi, A, Bonavera, L, Bond, JR, Borrill, J, Bouchet, FR, Boulanger, F, Burigana, C, Butler, RC, Calabrese, E, Catalano, A, Chiang, HC, Christensen, PR, Clements, DL, Colombo, LPL, Couchot, F, Coulais, A, Crill, BP, Curto, A, Cuttaia, F, Danese, L, Davies, RD, Davis, RJ, Bernardis, PD, Rosa, AD, Zotti, GD, Delabrouille, J, Dickinson, C, Diego, JM, Dole, H, Doré, O, Douspis, M, Ducout, A, Dupac, X, Elsner, F, Enßlin, TA, Eriksen, HK, Falgarone, E, Finelli, F, Flores-Cacho, I, Frailis, M, Fraisse, AA, Franceschi, E, Galeotta, S, Galli, S, Ganga, K, Giard, M, Giraud-Héraud, Y, Gjerløw, E, González-Nuevo, J, Górski, KM, Gregorio, A, Gruppuso, A, Gudmundsson, JE, Hansen, FK, Harrison, DL, Helou, G, Hernández-Monteagudo, C, Herranz, D, Hildebrandt, SR, Hivon, E, Hobson, M, Hornstrup, A, Hovest, W, Huffenberger, KM, Hurier, G, Jaffe, AH, Jaffe, TR, Keihänen, E, Keskitalo, R, Kisner, TS, Knoche, J, Kunz, M, Kurki-Suonio, H, Lagache, G, Lamarre, J-M, Lasenby, A, Lattanzi, M, Lawrence, CR, Leonardi, R, Levrier, F, Lilje, PB, Linden-Vørnle, M, López-Caniego, M, Lubin, PM, Macías-Pérez, JF, Maffei, B, Maggio, G, Maino, D, Mandolesi, N, Mangilli, A, Maris, M, Martin, PG, Martínez-González, E, Masi, S, Matarrese, S, Melchiorri, A, Mennella, A, Migliaccio, M, Mitra, S, Miville-Deschênes, M-A, Moneti, A, Montier, L, Morgante, G, Mortlock, D, Munshi, D, Murphy, JA, Nati, F, Natoli, P, Nesvadba, NPH, Noviello, F, Novikov, D, Novikov, I, Oxborrow, CA, Pagano, L, Pajot, F, Paoletti, D, Partridge, B, Pasian, F, Pearson, TJ, Perdereau, O, Perotto, L, Pettorino, V, Piacentini, F, Piat, M, Plaszczynski, S, Pointecouteau, E, Polenta, G, Pratt, GW, Prunet, S, Puget, J-L, Rachen, JP, Reinecke, M, Remazeilles, M, Renault, C, Renzi, A, Ristorcelli, I, Rocha, G, Rosset, C, Rossetti, M, Roudier, G, Rubiño-Martín, JA, Rusholme, B, Sandri, M, Santos, D, Savelainen, M, Savini, G, Scott, D, Spencer, LD, Stolyarov, V, Stompor, R, Sudiwala, R, Sunyaev, R, Suur-Uski, A-S, Sygnet, J-F, Tauber, JA, Terenzi, L, Toffolatti, L, Tomasi, M, Tristram, M, Tucci, M, Türler, M, Umana, G, Valenziano, L, Valiviita, J, Tent, BV, Vielva, P, Villa, F, Wade, LA, Wandelt, BD, Wehus, IK, Welikala, N, Yvon, D, Zacchei, A, Zonca, A
The Planck mission, thanks to its large frequency range and all-sky coverage, has a unique potential for systematically detecting the brightest, and rarest, submillimetre sources on the sky, including distant objects in the high-redshift Universe tra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1032::7aca82f2d3f44829798ea24244f104b3
http://hdl.handle.net/10044/1/39987
http://hdl.handle.net/10044/1/39987
Autor:
Bond, JR, Ade, P, Balbi, A, Bock, J, Borrill, J, Boscaleri, A, Coble, K, Crill, B, Bernardis, PD, Farese, P, Ferreira, P, Ganga, K, Giacometti, M, Hanany, S, Hivon, E, Hristov, V, Iacoangeli, A, Jaffe, A, Lange, A, Lee, A, Martinis, L, Masi, S, Mauskopf, P, Melchiorri, A, Montroy, T, Netterfield, B, Oh, S, Pascale, E, Piacentini, F, Pogosyan, D, Prunet, S, Rabii, B, Rao, S, Richards, P, Romeo, G, Ruhl, J, Scaramuzzi, F, Sforna, D, Sigurdson, K, Smoot, G, Stompor, R, Winant, C, Wu, P
We show how estimates of parameters characterizing inflation-based theories of structure formation localized over the past year when large scale structure (LSS) information from galaxy and cluster surveys was combined with the rapidly developing cosm
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::43c226da81f7f253860bfa8aa526ab01
https://ora.ox.ac.uk/objects/uuid:d3f55342-836e-436e-9323-7213b2c7500c
https://ora.ox.ac.uk/objects/uuid:d3f55342-836e-436e-9323-7213b2c7500c
Autor:
Hanany, S, Ade, P, Balbi, A, Bock, J, Borrill, J, Boscaleri, A, Bernardis, PD, Ferreira, PG, Hristov, VV, Jaffe, AH, Lange, AE, Lee, AT, Mauskopf, PD, Netterfield, CB, Oh, S, Pascale, E, Rabii, B, Richards, PL, Smoot, GF, Stompor, R, Winant, CD, Wu, JHP
We present a map and an angular power spectrum of the anisotropy of the cosmic microwave background (CMB) from the first flight of MAXIMA. MAXIMA is a balloon-borne experiment with an array of 16 bolometric photometers operated at 100 mK. MAXIMA obse
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::52f652900c8dcfe10294245a9697e14c
https://doi.org/10.1086/317322
https://doi.org/10.1086/317322
Autor:
Collaboration, PRISM, André, P, Baccigalupi, C, Banday, A, Barbosa, D, Barreiro, B, Bartlett, J, Bartolo, N, Battistelli, E, Battye, R, Bendo, G, Benoît, A, Bernard, JP, Bersanelli, M, Béthermin, M, Bielewicz, P, Bonaldi, A, Bouchet, FC, Boulanger, FC, Brand, J, Bucher, M, Burigana, C, Cai, ZY, Camus, P, Casas, F, Casasola, V, Castex, G, Challinor, A, Chluba, J, Chon, G, Colafrancesco, S, Comis, B, Cuttaia, F, D'Alessandro, G, Silva, AD, Davis, R, Avillez, MD, Bernardis, PD, Petris, MD, Rosa, AD, Zotti, GD, Delabrouille, J, Désert, FCX, Dickinson, C, Diego, JM, Dunkley, J, Enßlin, T, Errard, J, Falgarone, E, Ferreira, P, Ferrière, K, Finelli, F, Fletcher, A, Fosalba, P, Fuller, G, Galli, S, Ganga, K, García-Bellido, J, Ghribi, A, Giard, M, Giraud-Héraud, Y, Gonzalez-Nuevo, J, Grainge, K, Gruppuso, A, Hall, A, Hamilton, JC, Haverkorn, M, Hernandez-Monte-agudo, C, Herranz, D, Jackson, M, Jaffe, A, Khatri, R, Kunz, M, Lamagna, L, Lattanzi, M, Leahy, P, Lesgourgues, J, Liguori, M, Liuzzo, E, Lopez-Caniego, M, Macias-Perez, J, Maffei, B, Maino, D, Mangilli, A, Martinez-Gonzalez, E, Martins, C, Masi, S, Massardi, M, Matarrese, S, Melchiorri, A, Melin, JB, Mennella, A, Mignano, A, Miville-Deschênes, MA, Monfardini, A, Murphy, A, Naselsky, P, Nati, F, Natoli, P, Negrello, M, Noviello, F, O'Sullivan, C, Paci, F, Pagano, L, Paladino, R, Palanque-Delabrouille, N, Paoletti, D, Peiris, H, Perrotta, F, Piacentini, F, Piat, M, Piccirillo, L, Pisano, G, Polenta, G, Pollo, A, Ponthieu, N, Remazeilles, M, Ricciardi, S, Roman, M, Rosset, C, Rubino-Martin, JA, Salatino, M, Schillaci, A, Shellard, P, Silk, J, Starobinsky, A, Stompor, R, Sunyaev, R, Tartari, A, Terenzi, L, Toffolatti, L, Tomasi, M, Trappe, N, Tristram, M, Trombetti, T, Tucci, M, Weijgaert, RVD, Tent, BV, Verde, L, Vielva, P, Wandelt, B, Watson, R, Withington, S
Publikováno v:
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics, 2014, 02, pp.006. ⟨10.1088/1475-7516/2014/02/006⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Journal of Cosmology and Astroparticle Physics, 2014(02), 6-71. IOP PUBLISHING LTD
Journal of Cosmology and Astroparticle Physics, Institute of Physics (IOP), 2014, 02, pp.006. ⟨10.1088/1475-7516/2014/02/006⟩
Hall, A 2014, ' PRISM (Polarized Radiation Imaging and Spectroscopy Mission): an extended white paper ', Journal of Cosmology and Astroparticle Physics (JCAP), vol. 2014 . https://doi.org/10.1088/1475-7516/2014/02/006
Journal of Cosmology and Astroparticle Physics, 2014, 02, pp. 006(1)-006(20)
RUO. Repositorio Institucional de la Universidad de Oviedo
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Agência para a Sociedade do Conhecimento (UMIC)-FCT-Sociedade da Informação
instacron:RCAAP
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Journal of Cosmology and Astroparticle Physics, 2014, 006(1)-006(20)
Journal of Cosmology and Astroparticle Physics, 2014, 02, pp.006. ⟨10.1088/1475-7516/2014/02/006⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Journal of Cosmology and Astroparticle Physics, 2014(02), 6-71. IOP PUBLISHING LTD
Journal of Cosmology and Astroparticle Physics, Institute of Physics (IOP), 2014, 02, pp.006. ⟨10.1088/1475-7516/2014/02/006⟩
Hall, A 2014, ' PRISM (Polarized Radiation Imaging and Spectroscopy Mission): an extended white paper ', Journal of Cosmology and Astroparticle Physics (JCAP), vol. 2014 . https://doi.org/10.1088/1475-7516/2014/02/006
Journal of Cosmology and Astroparticle Physics, 2014, 02, pp. 006(1)-006(20)
RUO. Repositorio Institucional de la Universidad de Oviedo
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Agência para a Sociedade do Conhecimento (UMIC)-FCT-Sociedade da Informação
instacron:RCAAP
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Journal of Cosmology and Astroparticle Physics, 2014, 006(1)-006(20)
PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to ESA in May 2013 as a large-class mission for investigating within the framework of the ESA Cosmic Vision program a set of important scientific questions that require high re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d44469160a899f4bd050f8ff807faaf
http://hdl.handle.net/20.500.11767/15003
http://hdl.handle.net/20.500.11767/15003
Autor:
Bond, JR, Pogosyan, D, Prunet, S, Sigurdson, K, collaboration, TM, Ade, P, Balbi, A, Bock, J, Borrill, J, Boscaleri, A, Coble, K, Crill, B, Bernardis, PD, Farese, P, Ferreira, P, Ganga, K, Giacometti, M, Hanany, S, Hivon, E, Hristov, V, Iacoangeli, A, Jaffe, A, Lange, A, Lee, A, Martinis, L, Masi, S, Mauskopf, P, Melchiorri, A, Montroy, T, Netterfield, B, Oh, S, Pascale, E, Piacentini, F, Rabii, B, Rao, S, Richards, P, Romeo, G, Ruhl, J, Scaramuzzi, F, Sforna, D, Smoot, G, Stompor, R, Winant, C, Wu, P
The past, present and future of cosmic microwave background (CMB) anisotropy research is discussed, with emphasis on the Boomerang and Maxima balloon experiments. These data are combined with large scale structure (LSS) information and high redshift
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1064::5e0d101ff5a4c060079f73d572a14bd9
http://ora.ox.ac.uk/objects/uuid:47bd84aa-1b19-4fe2-868a-58eaa49140dd
http://ora.ox.ac.uk/objects/uuid:47bd84aa-1b19-4fe2-868a-58eaa49140dd